Spitzer对北黄极的观测
星系天体物理
2018-02-21 v1
摘要
我们给出了Spitzer空间望远镜对北黄极(NEP;中心位于 , )暖任务观测的光度星表。观测使用IRAC在3.6 m和4.5 m波段进行,覆盖面积7.04 deg,在3.6 m和4.5 m波段分别达到1深度1.29 Jy和0.79 Jy。该光度星表包含全深度NEP mosaic上具有3.6 m和4.5 m波段测光的380,858个源。点源完备性模拟表明该星表在19.7 AB星等下完备度为80%。随附星表可用于约束河外天体的物理性质、研究AGN族、测量恒星天体的红外颜色以及研究河外红外背景光。
引用
@article{arxiv.1712.01290,
title = {Spitzer Observations of the North Ecliptic Pole},
author = {H. Nayyeri and N. Ghotbi and A. Cooray and J. Bock and D. L. Clements and M. Im and M. G. Kim and P. Korngut and A. Lanz and H. M. Lee and D. H. Lee and M. Malkan and H. Matsuhara and T. Matsumoto and S. Matsuura and U. W. Nam and C. Pearson and S. Serjeant and J. Smidt and K. Tsumura and T. Wada and M. Zemcov},
journal= {arXiv preprint arXiv:1712.01290},
year = {2018}
}
备注
10 pages, 11 figures and 3 tables. Accepted to the ApJS